Magma Ocean Processes

Magma Ocean Processes is a planetary-scale geophysical phenomenon characterized by the widespread melting and convective differentiation of primordial silicate materials during the early accretion phase of terrestrial planet formation.

477

Publications

37.7K

Citations

1.3K

Authors

523

Institutions

Publications per year

2017–2026

163

Authors

1.3K

  1. LT
    L. T. Elkins‐Tanton

    Massachusetts Institute of Technology, United States

    15 publications · 2.2K citations

    15

    h-index

  2. YA
    Yutaka Abe

    The University of Tokyo, Japan

    9 publications · 1.4K citations

    9

    h-index

  3. FN
    F. Nimmo

    University of California, Santa Cruz, United States

    8 publications · 449 citations

    8

    h-index

  4. DC
    D. C. Rubie

    University of Bayreuth, Germany

    8 publications · 1K citations

    8

    h-index

  5. DB
    D. Breuer

    Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR), Germany

    6 publications · 336 citations

    6

    h-index

1–5 of 1.3K

Venues

  1. Earth and Planetary Science Letters

    71 publications · 6.1K citations

    44

    h-index

  2. Geochimica et Cosmochimica Acta

    26 publications · 1.7K citations

    22

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 19 publications · 2.3K citations

    18

    h-index

  4. Nature

    18 publications · 4.1K citations

    18

    h-index

  5. Journal of Geophysical Research Planets

    16 publications · 1.4K citations

    16

    h-index

1–5